Unified Astronomy Thesaurus
Toggle navigation
Home
Advanced search
About...
My account
Observational astronomy
Home
Observational astronomy
Term
Metadata
Observational astronomy
Alternative terms
UF
↸
Imaging of stars
UF
↸
Stellar imaging
More specific terms
NT1
↓
Amateur astronomy
NT1
↓
Astronomical location
►
▼
NT2
↓
Line of sight
NT2
↓
Location behind
NT2
↓
Location between
NT2
↓
Location in front
NT1
↓
Astronomical object identification
NT1
↓
Astronomical optics
►
▼
NT2
↓
Astronomical seeing
NT2
↓
Atmospheric refraction
NT2
↓
Atmospheric scintillation
►
▼
NT3
↓
Ionospheric scintillation
NT2
↓
Collimation
NT2
↓
Dark adaption
NT2
↓
Extinction
►
▼
NT3
↓
Atmospheric extinction
►
▼
NT4
↓
Ultraviolet extinction
NT3
↓
Interstellar extinction
►
▼
NT4
↓
Interstellar reddening
NT2
↓
Interplanetary scintillation
NT2
↓
Interstellar scintillation
NT2
↓
Laser guide stars
NT2
↓
Stellar atmospheric opacity
NT1
↓
Astronomical site protection
NT1
↓
Astronomical spectroscopy
►
▼
NT2
↓
Lyman alpha forest
NT1
↓
Astronomical transits
NT1
↓
Astrophotography
►
▼
NT2
↓
Darkrooms
NT2
↓
Remote telescope astrophotography
NT2
↓
Telescope focal plane photography
NT1
↓
Axial tilt
NT1
↓
Blinking
NT1
↓
Bright point
NT1
↓
Coronographic imaging
NT1
↓
Cosmic background radiation
►
▼
NT2
↓
Cosmic microwave background radiation
NT2
↓
Sunyaev-Zeldovich effect
NT1
↓
Cosmic ray astronomy
NT1
↓
Doppler imaging
NT1
↓
Doppler shift
►
▼
NT2
↓
Blueshift
NT2
↓
Redshift
NT1
↓
Drift scan imaging
NT1
↓
Extrasolar planet detection
NT1
↓
Field of view
NT1
↓
Finding charts
NT1
↓
Finding lists
NT1
↓
Gamma-ray astronomy
NT1
↓
Gravitational wave astronomy
NT1
↓
Ground-based astronomy
NT1
↓
Heliocentric correction
NT1
↓
High angular resolution
NT1
↓
High energy astronomy
NT1
↓
High time resolution astrophysics
NT1
↓
Infrared astronomy
►
▼
NT2
↓
Far infrared astronomy
NT2
↓
Far-infrared astronomy
NT2
↓
Infrared excess
NT2
↓
Near infrared astronomy
NT1
↓
Limb brightening
NT1
↓
Limb darkening
NT1
↓
Magnitude
►
▼
NT2
↓
Absolute magnitude
►
▼
NT3
↓
Wilson-Bappu Effect
NT2
↓
Apparent magnitude
►
▼
NT3
↓
B magnitude
NT3
↓
H magnitude
NT3
↓
I magnitude
NT3
↓
J magnitude
NT3
↓
K magnitude
NT3
↓
L magnitude
NT3
↓
Limiting magnitude
NT3
↓
M magnitude
NT3
↓
N magnitude
NT3
↓
O magnitude
NT3
↓
P magnitude
NT3
↓
Period determination
NT3
↓
Photoelectric magnitude
NT3
↓
Photographic magnitude
NT3
↓
Photovisual magnitude
NT3
↓
Pogson scale
NT3
↓
Q magnitude
NT3
↓
R magnitude
NT3
↓
Two-color diagrams
NT3
↓
U magnitude
NT3
↓
V magnitude
NT3
↓
Variable star period change
NT2
↓
Integrated magnitude
NT1
↓
Meridian observation
NT1
↓
Neutrino astronomy
►
▼
NT2
↓
Neutrino masses
NT2
↓
Solar neutrino problem
NT2
↓
Urca process
NT1
↓
Observation techniques
►
▼
NT2
↓
Astrometry
►
▼
NT3
↓
Angular separation
NT3
↓
Astronomical unit
NT3
↓
Baade-Wesselink method
NT3
↓
Bolometric correction
NT3
↓
Brightness temperature
NT3
↓
Cosmic ray detectors
NT3
↓
Dark matter detectors
NT3
↓
Effective temperature
NT3
↓
Equator position
NT3
↓
Fundamental parameters of stars
NT3
↓
Light year
NT3
↓
Luminosity function
NT3
↓
Parsec
NT3
↓
Photographic astrometry
►
▼
NT4
↓
Photogrammetry
NT3
↓
Radial velocity
NT3
↓
Radio astrometry
NT3
↓
Relaxation time
NT3
↓
Sky noise
NT3
↓
Space astrometry
NT3
↓
Spectral index
NT3
↓
Standard stars
►
▼
NT4
↓
Comparison stars
NT4
↓
Photometric standard stars
NT3
↓
Stellar distance
►
▼
NT4
↓
Cepheid distance
NT4
↓
Distance indicators
NT4
↓
Faber-Jackson distance
NT4
↓
Standard candles
NT3
↓
Two-color diagrams
NT3
↓
Wolf diagram
NT2
↓
CCD observation
NT2
↓
Interferometry
►
▼
NT3
↓
Adaptive interferometry
NT3
↓
Aperture synthesis
NT3
↓
Atom interferometry
NT3
↓
Direct detection interferometry
NT3
↓
Heterodyne interferometry
NT3
↓
Holographic interferometry
NT3
↓
Interferometric correlation
NT3
↓
Laser interferometry
►
▼
NT4
↓
LIGO
NT3
↓
Long baseline interferometry
NT3
↓
Neutron interferometry
NT3
↓
Nonclassical interferometry
NT3
↓
Optical interferometry
►
▼
NT4
↓
Optical phase shifting interferometry
►
NT3
↓
Phase switching
NT3
↓
Radio interferometry
►
▼
NT4
↓
Very long baseline interferometry
NT3
↓
Speckle interferometry
NT3
↓
Visibility function
NT2
↓
Night vision
NT2
↓
Optical observation
NT2
↓
Photometry
►
▼
NT3
↓
CCD photometry
►
▼
NT4
↓
Broad band photometry
►
NT4
↓
Medium band photometry
►
NT4
↓
Narrow band photometry
►
NT3
↓
Color equations
NT3
↓
Galaxy photometry
NT3
↓
Infrared photometry
NT3
↓
Light curves
NT3
↓
Multi-color photometry
NT3
↓
Photoelectric photometry
►
▼
NT4
↓
Broad band photometry
►
NT4
↓
Medium band photometry
►
NT4
↓
Narrow band photometry
►
NT3
↓
Photographic photometry
►
▼
NT4
↓
Broad band photometry
►
NT4
↓
Photogrammetry
NT3
↓
Photometric standard stars
NT3
↓
Photometric systems
►
▼
NT4
↓
Bessel photometry
NT4
↓
Cape photometry
NT4
↓
DDO photometry
NT4
↓
Geneva photometry
NT4
↓
Gunn photometry
NT4
↓
HST photometry
NT4
↓
Johnson photometry
NT4
↓
Kron-Cousins photometry
NT4
↓
RGB photometry
NT4
↓
Sloan photometry
NT4
↓
Strömgren photometric system
NT4
↓
Walraven photometry
NT3
↓
Spectrophotometry
NT3
↓
Surface photometry
NT3
↓
Two-color diagrams
NT3
↓
Ultraviolet photometry
►
▼
NT4
↓
Ultraviolet color
NT2
↓
Polarimetry
NT1
↓
Observational cosmology
►
▼
NT2
↓
Cosmological constant
►
▼
NT3
↓
Cosmological constant experiments
NT2
↓
Hubble constant
NT1
↓
Observatories
►
▼
NT2
↓
Antarctic observatories
NT2
↓
Domes
NT2
↓
Gamma-ray observatories
NT2
↓
Infrared observatories
►
▼
NT3
↓
Infrared Astronomical Satellite
NT2
↓
Optical observatories
►
▼
NT3
↓
Hubble Space Telescope
NT2
↓
Radio observatories
NT2
↓
Solar observatories
NT2
↓
Space observatories
►
▼
NT3
↓
Gamma-ray observatories
NT3
↓
Hubble Space Telescope
NT3
↓
Infrared Astronomical Satellite
NT2
↓
Ultraviolet observatories
►
▼
NT3
↓
Hubble Space Telescope
NT2
↓
X-ray observatories
NT1
↓
Occultation
►
▼
NT2
↓
Asteroid occultation
NT2
↓
Eclipses
►
▼
NT3
↓
Annular eclipses
NT3
↓
Antumbra
NT3
↓
Baily's beads
NT3
↓
Lunar eclipses
►
▼
NT4
↓
Saros cycle
NT3
↓
Partial eclipses
NT3
↓
Penumbra
NT3
↓
Solar eclipses
►
▼
NT4
↓
Diamond ring effect
NT4
↓
Flash spectra
NT4
↓
Shadow bands
NT3
↓
Total eclipses
NT3
↓
Umbra
NT3
↓
Zone of totality
NT2
↓
Lunar occultation
NT2
↓
Occulting disks
NT2
↓
Radio occultation
NT1
↓
Optical doubles
NT1
↓
Optical identification
NT1
↓
Photometry
►
▼
NT2
↓
CCD photometry
►
▼
NT3
↓
Broad band photometry
►
▼
NT4
↓
Bessel photometry
NT4
↓
BV photometry
NT4
↓
Cape photometry
NT4
↓
Cape RI photometry
NT4
↓
Gunn photometry
NT4
↓
HST photometry
NT4
↓
Johnson photometry
NT4
↓
Kron-Cousins photometry
NT4
↓
RGB photometry
NT4
↓
RGU photometry
NT4
↓
Sloan photometry
NT4
↓
Two-color photometry
►
NT4
↓
Ultraviolet photometry
►
NT3
↓
Medium band photometry
►
▼
NT4
↓
DDO photometry
NT4
↓
Geneva photometry
NT4
↓
Strömgren photometric system
NT4
↓
Ultraviolet photometry
►
NT4
↓
Vilnius photometry
NT4
↓
Walraven photometry
NT3
↓
Narrow band photometry
►
▼
NT4
↓
H alpha photometry
NT4
↓
H beta photometry
NT2
↓
Color equations
NT2
↓
Galaxy photometry
NT2
↓
Infrared photometry
NT2
↓
Light curves
NT2
↓
Multi-color photometry
NT2
↓
Photoelectric photometry
►
▼
NT3
↓
Broad band photometry
►
▼
NT4
↓
Bessel photometry
NT4
↓
BV photometry
NT4
↓
Cape photometry
NT4
↓
Cape RI photometry
NT4
↓
Gunn photometry
NT4
↓
HST photometry
NT4
↓
Johnson photometry
NT4
↓
Kron-Cousins photometry
NT4
↓
RGB photometry
NT4
↓
RGU photometry
NT4
↓
Sloan photometry
NT4
↓
Two-color photometry
►
NT4
↓
Ultraviolet photometry
►
NT3
↓
Medium band photometry
►
▼
NT4
↓
DDO photometry
NT4
↓
Geneva photometry
NT4
↓
Strömgren photometric system
NT4
↓
Ultraviolet photometry
►
NT4
↓
Vilnius photometry
NT4
↓
Walraven photometry
NT3
↓
Narrow band photometry
►
▼
NT4
↓
H alpha photometry
NT4
↓
H beta photometry
NT2
↓
Photographic photometry
►
▼
NT3
↓
Broad band photometry
►
▼
NT4
↓
Bessel photometry
NT4
↓
BV photometry
NT4
↓
Cape photometry
NT4
↓
Cape RI photometry
NT4
↓
Gunn photometry
NT4
↓
HST photometry
NT4
↓
Johnson photometry
NT4
↓
Kron-Cousins photometry
NT4
↓
RGB photometry
NT4
↓
RGU photometry
NT4
↓
Sloan photometry
NT4
↓
Two-color photometry
►
NT4
↓
Ultraviolet photometry
►
NT3
↓
Photogrammetry
NT2
↓
Photometric standard stars
NT2
↓
Photometric systems
►
▼
NT3
↓
Bessel photometry
NT3
↓
Cape photometry
NT3
↓
DDO photometry
NT3
↓
Geneva photometry
NT3
↓
Gunn photometry
NT3
↓
HST photometry
NT3
↓
Johnson photometry
NT3
↓
Kron-Cousins photometry
NT3
↓
RGB photometry
NT3
↓
Sloan photometry
NT3
↓
Strömgren photometric system
NT3
↓
Walraven photometry
NT2
↓
Spectrophotometry
NT2
↓
Surface photometry
NT2
↓
Two-color diagrams
NT2
↓
Ultraviolet photometry
►
▼
NT3
↓
Ultraviolet color
NT1
↓
Pointing accuracy
►
▼
NT2
↓
Pointing error
NT1
↓
Purkinje effect
NT1
↓
Radar astronomy
NT1
↓
Radio astronomy
►
▼
NT2
↓
Brightness temperature
NT2
↓
Cosmic noise
►
▼
NT3
↓
Cosmic microwave background radiation
NT2
↓
Interplanetary scintillation
NT2
↓
Interstellar scintillation
NT2
↓
Millimeter astronomy
NT2
↓
Radio astrometry
NT2
↓
Radio spectroscopy
NT2
↓
Spectral index
NT2
↓
Submillimeter astronomy
NT2
↓
Sunyaev-Zeldovich effect
NT1
↓
Reddening
►
▼
NT2
↓
Interstellar reddening
NT2
↓
Reddened stars
NT2
↓
Reddening law
NT1
↓
Ultraviolet astronomy
►
▼
NT2
↓
Near ultraviolet astronomy
NT1
↓
Visible astronomy
NT1
↓
Visual observation
NT1
↓
X-ray astronomy
►
▼
NT2
↓
X-ray bright point
NT2
↓
X-ray identification
NT1
↓
Zeeman–Doppler imaging
NT1
↓
Zenith hourly rate
Related terms
RT
⇆
Telescopes
Date of creation
18-Dec-2013
Accepted term
18-Dec-2013
Descendant terms
150
ARK
ark:/99152/t339dr0m780e1w
More specific terms
52
Alternative terms
2
Related terms
1
Notes
0
Metadata
BS8723-5
DC
MADS
SKOS-Core
VDEX
XTM
Zthes
JSON
JSON-LD
Search
Central terms
Observatories
Radio astronomy
Astronomical optics
Occultation
Infrared astronomy
Astronomical location
Astrophotography
Cosmic background radiation
Magnitude
Neutrino astronomy